To the Schwarzschild Solution in General Relativity  

作　　者：Valery V. Vasiliev Leonid V. Fedorov 

机构地区：[1]Institute of Problems in Mechanics, Russian Academy of Sciences, Moscow, Russia

出　　处：《Journal of Modern Physics》2018年第14期2482-2494,共13页现代物理（英文）

摘　　要：The paper is concerned with the history of the spherically symmetric static problem solution of General Relativity found in 1916 by K. Schwarzschild [1] [2] which is interpreted in modern physics as the background of the objects referred to as Black Holes. First, the modern interpretation this solution which does not exactly coincide with original solution obtained by K. Schwarzschild is discussed. Second, the basic equations of the original Schwarzschild solution are presented in modern notations allowing us to compare existing and original solutions. Finally, a modification of the Schwarzschild approach is proposed allowing us to arrive at the exact solution of the Schwarzschild problem.The paper is concerned with the history of the spherically symmetric static problem solution of General Relativity found in 1916 by K. Schwarzschild [1] [2] which is interpreted in modern physics as the background of the objects referred to as Black Holes. First, the modern interpretation this solution which does not exactly coincide with original solution obtained by K. Schwarzschild is discussed. Second, the basic equations of the original Schwarzschild solution are presented in modern notations allowing us to compare existing and original solutions. Finally, a modification of the Schwarzschild approach is proposed allowing us to arrive at the exact solution of the Schwarzschild problem.

关 键 词：General RELATIVITY Spherically SYMMETRIC Problem Schwarzschild’s SOLUTION Black HOLES 

分 类 号：O1[理学—数学]